Broad Band Photometry of the Solar Corona of 1983, June 11

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/399

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DC Field	Value	Language
dc.contributor.author	Sivaraman, K. R	-
dc.contributor.author	Singh, J	-
dc.contributor.author	Kapoor, R. C	-
dc.contributor.author	Kariyappa, R	-
dc.date.accessioned	2005-05-18T07:01:54Z	-
dc.date.available	2005-05-18T07:01:54Z	-
dc.date.issued	1985-11	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 5, No. 1, pp. 31-36	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/399	-
dc.description.abstract	The solar corona was photographed at an effective wavelength of 6300A during the total eclipse of 1983, June 11 at Indonesia. From the isophotes of the corona, the intensity distributions along the equator, poles, streamers and gaps have been derived. The intensity along the equatorial and polar directions can be represented well by a 19/sup0/ polynomial. The brightness distribution and the Ludendorff parameters of this corona are typical of the intermediate phase of the solar cycle	en
dc.format.extent	173302 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar Corona	en
dc.subject	Solar Eclipse	en
dc.subject	Coronal Photometry	en
dc.title	Broad Band Photometry of the Solar Corona of 1983, June 11	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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